The Active Galactic Nuclei in the Hobby-Eberly Telescope Dark Energy Experiment Survey (HETDEX). III. A Red Quasar with Extremely High Equivalent Widths Showing Powerful Outflows
dc.bibliographicCitation.firstPage | 40 | |
dc.bibliographicCitation.issue | 1 | |
dc.bibliographicCitation.journalTitle | The Astrophysical Journal | eng |
dc.bibliographicCitation.volume | 940 | |
dc.contributor.author | Liu, Chenxu | |
dc.contributor.author | Gebhardt, Karl | |
dc.contributor.author | Kollatschny, Wolfram | |
dc.contributor.author | Ciardullo, Robin | |
dc.contributor.author | Mentuch Cooper, Erin | |
dc.contributor.author | Davis, Dustin | |
dc.contributor.author | Farrow, Daniel J. | |
dc.contributor.author | Finkelstein, Steven L. | |
dc.contributor.author | Gawiser, Eric | |
dc.contributor.author | Gronwall, Caryl | |
dc.contributor.author | Hill, Gary J. | |
dc.contributor.author | House, Lindsay | |
dc.contributor.author | Schneider, Donald P. | |
dc.contributor.author | Urrutia, Tanya | |
dc.contributor.author | Zeimann, Gregory R. | |
dc.date.accessioned | 2023-02-06T08:02:53Z | |
dc.date.available | 2023-02-06T08:02:53Z | |
dc.date.issued | 2022 | |
dc.description.abstract | We report an active galactic nucleus (AGN) with an extremely high equivalent width (EW), EWLyα+N V,rest ≳921 Å, in the rest frame, at z ∼ 2.24 in the Hobby-Eberly Telescope Dark Energy Experiment Survey (HETDEX), as a representative case of the high-EW AGN population. The continuum level is a nondetection in the HETDEX spectrum; thus the measured EW is a lower limit. The source is detected with significant emission lines (>7σ) at Lyα + N v λ1241, C iv λ1549, and a moderate emission line (∼4σ) at He ii λ1640 within the wavelength coverage of HETDEX (3500-5500 Å). The r-band magnitude is 24.57 from the Hyper Suprime-Cam-HETDEX joint survey with a detection limit of r = 25.12 at 5σ. The Lyα emission line spans a clearly resolved region of ∼10″ (85 kpc) in diameter. The Lyα line profile is strongly double peaked. The spectral decomposed blue gas and red gas Lyα emission are separated by ∼1.″2 (10.1 kpc) with a line-of-sight velocity offset of ∼1100 km s−1. This source is probably an obscured AGN with powerful winds. | eng |
dc.description.version | publishedVersion | eng |
dc.identifier.uri | https://oa.tib.eu/renate/handle/123456789/11246 | |
dc.identifier.uri | http://dx.doi.org/10.34657/10282 | |
dc.language.iso | eng | |
dc.publisher | London : Institute of Physics Publ. | |
dc.relation.doi | https://doi.org/10.3847/1538-4357/ac9af2 | |
dc.relation.essn | 1538-4357 | |
dc.relation.issn | 0004-637X | |
dc.rights.license | CC BY 4.0 Unported | |
dc.rights.uri | https://creativecommons.org/licenses/by/4.0 | |
dc.subject.ddc | 520 | |
dc.subject.other | images | eng |
dc.subject.other | galaxy | eng |
dc.subject.other | sky | eng |
dc.title | The Active Galactic Nuclei in the Hobby-Eberly Telescope Dark Energy Experiment Survey (HETDEX). III. A Red Quasar with Extremely High Equivalent Widths Showing Powerful Outflows | eng |
dc.type | Article | eng |
dc.type | Text | eng |
tib.accessRights | openAccess | |
wgl.contributor | AIP | |
wgl.subject | Physik | ger |
wgl.type | Zeitschriftenartikel | ger |
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